Iqueye, a single photon-counting photometer applied to the ESO new technology telescope

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Table 3:

Values of $\langle g^{(2)}(d) \rangle$ obtained from one hour observation of the bright star $\zeta$ Ori, for each pair a,bof sub-apertures, assuming a time coincidence window $\Delta t = 244.1$ ps.
Channel pair	Effective distance	Resolving angle	$\langle g^{(2)}(d) \rangle$	Standard
(channel numbers)	d (m)	$\theta$ (arcsec)		deviation
A-B	1.7	0.052	0.886	0.002
A-C	2.4	0.037	0.912	0.003
A-D	1.7	0.052	0.931	0.001
B-C	1.7	0.052	0.909	0.002
B-D	2.4	0.037	0.909	0.004
C-D	1.7	0.052	0.932	0.004

Source LaTeX | All tables | In the text

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